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1. Identity statement
Reference TypeJournal Article
Sitemtc-m21c.sid.inpe.br
Holder Codeisadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S
Identifier8JMKD3MGP3W34R/3UME4RH
Repositorysid.inpe.br/mtc-m21c/2020/01.03.14.49   (restricted access)
Last Update2020:01.03.14.49.53 (UTC) simone
Metadata Repositorysid.inpe.br/mtc-m21c/2020/01.03.14.49.53
Metadata Last Update2020:01.06.22.09.19 (UTC) administrator
DOI10.1007/s11207-019-1568-6
ISSN0038-0938
1573-093X
Citation KeySelhorstKalCasValCos:2019:SoRa37
TitleThe solar radius at 37 GHz through cycles 22 to 24
Year2019
MonthNov.
Access Date2024, May 17
Type of Workjournal article
Secondary TypePRE PI
Number of Files1
Size1153 KiB
2. Context
Author1 Selhorst, Caius L.
2 Kallunki, Juha
3 Castro, Carlos Guillermo Giménez de
4 Valio, Adriana
5 Costa, Joaquim Eduardo Rezende
Resume Identifier1
2
3
4
5 8JMKD3MGP5W/3C9JHF8
ORCID1 0000-0002-5897-5236
2 0000-0002-0325-5565
3 0000-0002-8979-3582
4 0000-0002-1671-8370
5 0000-0002-0703-4735
Group1
2
3
4
5 DIDAS-CGCEA-INPE-MCTIC-GOV-BR
Affiliation1 Universidade Cruzeiro do Sul
2 Metsähovi Radio Observatory
3 Universidade Presbiteriana Mackenzie
4 Universidade Presbiteriana Mackenzie
5 Instituto Nacional de Pesquisas Espaciais (INPE)
Author e-Mail Address1
2
3
4
5 joaquim.costa@inpe.br
JournalSolar Physics
Volume294
Number12
Pagese175
Secondary MarkA2_INTERDISCIPLINAR A2_GEOCIÊNCIAS A2_BIOTECNOLOGIA B1_ENGENHARIAS_IV B1_ASTRONOMIA_/_FÍSICA B2_CIÊNCIA_DA_COMPUTAÇÃO
History (UTC)2020-01-03 14:49:53 :: simone -> administrator ::
2020-01-03 14:49:54 :: administrator -> simone :: 2019
2020-01-03 14:50:39 :: simone -> administrator :: 2019
2020-01-06 22:09:19 :: administrator -> simone :: 2019
3. Content and structure
Is the master or a copy?is the master
Content Stagecompleted
Transferable1
Content TypeExternal Contribution
Version Typepublisher
KeywordsSun: radio radiation · Solar cycle · Sun: radius
AbstractTo better understand the influence of the activity cycle on the solar atmosphere, we report the time variation of the radius observed at 37 GHz (λ = 8.1 mm) obtained by the Metsähovi Radio Observatory (MRO) through Solar Cycles 22 to 24 (1989 2015). Almost 5800 maps were analyzed, however, due to instrumental setup changes the dataset showed four distinct behaviors, which required a normalization process to allow for the whole interval analysis. When the whole period was considered, the results showed a positive correlation index of 0.17 between the monthly means of the solar radius at 37 GHz and solar flux obtained at 10.7 cm (F10.7). This correlation index increased to 0.44, when only the data obtained during the last period without instrumental changes were considered (1999 2015). The solar radius correlation with the solar cycle agrees with the previous results obtained at mm/cm wavelengths (17 and 48 GHz), nevertheless, this result is the opposite of that reported at submillimeter wavelengths (212 and 405 GHz).
AreaCEA
Arrangementurlib.net > BDMCI > Fonds > Produção anterior à 2021 > DIDAS > The solar radius...
doc Directory Contentaccess
source Directory Contentthere are no files
agreement Directory Content
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4. Conditions of access and use
Languageen
Target Fileselhorst_solar.pdf
User Groupsimone
Reader Groupadministrator
simone
Visibilityshown
Archiving Policydenypublisher denyfinaldraft12
Read Permissiondeny from all and allow from 150.163
Update Permissionnot transferred
5. Allied materials
Mirror Repositoryurlib.net/www/2017/11.22.19.04.03
Next Higher Units8JMKD3MGPCW/3ETR8EH
Citing Item Listsid.inpe.br/bibdigital/2013/10.01.00.07 6
sid.inpe.br/mtc-m21/2012/07.13.14.51.06 1
DisseminationWEBSCI; PORTALCAPES; SCOPUS.
Host Collectionurlib.net/www/2017/11.22.19.04
6. Notes
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